Core Mass Estimates in Strong Lensing Galaxy Clusters: A Comparison between Masses Obtained from Detailed Lens Models, Single-halo Lens Models, and Einstein Radii

The core mass of galaxy clusters is both an important anchor of the radial mass distribution profile and a probe of structure formation. With thousands of strong lensing galaxy clusters being discovered by current and upcoming surveys, timely, efficient, and accurate core mass estimates are needed....

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Veröffentlicht in:	The Astrophysical journal 2021-10, Vol.920 (2), p.98
Hauptverfasser:	Remolina González, J. D., Sharon, K., Mahler, G., Fox, C., Garcia Diaz, C. A., Napier, K., Bleem, L. E., Gladders, M. D., Li, N., Niemiec, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models ASTRONOMY AND ASTROPHYSICS Astrophysics Cosmology: Dark Matter Estimates Galactic clusters Galaxies Galaxies: Clusters: General Galaxy clusters Galaxy distribution Gravitational Lensing: Strong Ionization Lenses Mass distribution Polls & surveys Stars & galaxies Strong gravitational lensing Supernova
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